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Energy of a nucleus
Energy of a nucleus

Fission and Fusion Power Point
Fission and Fusion Power Point

NUCLEAR CHEMISTRY
NUCLEAR CHEMISTRY

Nuclear Fission and Nuclear Fusion
Nuclear Fission and Nuclear Fusion

Lecture 30/3 Nuclear processes Ulf Torkelsson 1 Nuclear reactions
Lecture 30/3 Nuclear processes Ulf Torkelsson 1 Nuclear reactions

... nucleon decreases with the size of the nucleus. Therefore there are two ways of deriving energy from atomic nuclei, by fusing light nuclei, and by fissioning heavy nuclei. The nuclei that are involved in a fusion reaction are repelling each other through the Coulomb force, since they are both positi ...
Click here for printer-friendly sample test questions
Click here for printer-friendly sample test questions

Nuclear Reactions
Nuclear Reactions

... The missing mass (mass defect) has been stored as energy in the nucleus. It is called the binding energy of the nucleus. ...
Unit #12: Nuclear Chemistry
Unit #12: Nuclear Chemistry

... DON’T COPY: Radioactive C-14 is formed in the upper atmosphere by nuclear reactions initiated by neutrons in cosmic radiation 14N + 1 n ---> 14C + 1H ...
Fission and Fusion
Fission and Fusion

... In this example, a stray neutron strikes an atom of U-235. It absorbs the neutron and becomes an unstable atom of U-236. It then undergoes fission. Notice that more neutrons are released in the reaction. These neutrons can strike other U-235 atoms to initiate their fission. ...
NUCLEAR CHEMISTRY
NUCLEAR CHEMISTRY

Fusion or Fission
Fusion or Fission

... get it started. In the right conditions, it can sustain itself, once started. One of the benefits of fusion reactions is that there are no radioactive byproducts. On earth, fusion reactions result in the element helium. Heavier elements, like beryllium or carbon, are produced by fusion in stars. Hyd ...
nuclear fusion
nuclear fusion

By what process do most stars release energy? A. Electromagnetic
By what process do most stars release energy? A. Electromagnetic

Atom and Nucleus. Radioactivity. Nuclear Energy.
Atom and Nucleus. Radioactivity. Nuclear Energy.

... Ernest Rutherford attempted to test this model by bombarding a thin gold foil with alpha-particles. A significant scattering of the alpha-particles was ...
Nuclear Reactions Review
Nuclear Reactions Review

... 3.Nuclei with too many or too few neutrons are A.never found. C.unnatural. B.unstable. D.stable. ...
Nuclear Reactions Review powerpt
Nuclear Reactions Review powerpt

... 3.Nuclei with too many or too few neutrons are A.never found. C.unnatural. B.unstable. D.stable. ...
Nuclear Power Date
Nuclear Power Date

Physical Science: Nuclear Chemistry Study Guide
Physical Science: Nuclear Chemistry Study Guide

Summative Assessment Review!
Summative Assessment Review!

Nuclear Fission and Fusion
Nuclear Fission and Fusion

... 1) If a radioactive sample of rock started with 100 counts per second and 2 hours later has a count rate of 25 counts per second, what is it’s half-life? Try these questions, have a go at the answer 1) What do you think is meant by a ‘chain reaction?’ 2) The gold that exists on our planet, where did ...
Document
Document

... 1. The amount of material left after two half-lives is _one-fourth (1/4) _ of the original amount. 2. _Fission_ means "to divide." 3. _Nuclear Fusion_ is the combining of two low-mass nuclei into one nucleus with a larger mass. 4. Radioactive isotopes that are put into the body to monitor a bodily p ...
Nuclear Fission and Fusion Notes
Nuclear Fission and Fusion Notes

File
File

1.6--NOTES--Detecting Radiation Nuclear Rxtns
1.6--NOTES--Detecting Radiation Nuclear Rxtns

... The nuclear reaction that splits large nuclei into 2 smaller nuclei is (fission, fusion). ...
Fission and Fusion
Fission and Fusion

... • In controlled fission water or graphite are used to absorb some of the neutrons produced by fission, controlling the rate of the fission process. • Fusion is the fusing of two unstable hydrogen atoms to form helium. • Fusion is harder to start and control than fission, but produces more energy per ...
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Muon-catalyzed fusion

Muon-catalyzed fusion (μCF) is a process allowing nuclear fusion to take place at temperatures significantly lower than the temperatures required for thermonuclear fusion, even at room temperature or lower. It is one of the few known ways of catalyzing nuclear fusion reactions.Muons are unstable subatomic particles. They are similar to electrons, but are about 207 times more massive. If a muon replaces one of the electrons in a hydrogen molecule, the nuclei are consequently drawn 207 times closer together than in a normal molecule. When the nuclei are this close together, the probability of nuclear fusion is greatly increased, to the point where a significant number of fusion events can happen at room temperature.Current techniques for creating large numbers of muons require large amounts of energy, larger than the amounts produced by the catalyzed nuclear fusion reactions. This prevents it from becoming a practical power source. Moreover, each muon has about a 1% chance of ""sticking"" to the alpha particle produced by the nuclear fusion of a deuterium with a tritium, removing the ""stuck"" muon from the catalytic cycle, meaning that each muon can only catalyze at most a few hundred deuterium tritium nuclear fusion reactions. So, these two factors, of muons being too expensive to make and then sticking too easily to alpha particles, limit muon-catalyzed fusion to a laboratory curiosity. To create useful room-temperature muon-catalyzed fusion reactors would need a cheaper, more efficient muon source and/or a way for each individual muon to catalyze many more fusion reactions.
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